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Cosmic Mysteries Revealed: The Short and Brilliant Lives of Compressed Compact Objects

A new study reveals details of an unknown class of galaxies called compact compact objects (CSOs) that emit jets moving in opposite directions at speeds close to the speed of light

A new study of an unknown class of galaxies called compact compact objects (CSOs) reveals that these objects are not quite what they seem. CSOs are active galaxies centered on a supermassive black hole. From these monstrous black holes emerge two jets moving in opposite directions at a speed close to the speed of light. But compared to other galaxies that emit intense jets, these jets do not extend to great distances - they are much more compact. For decades scientists thought that CSOs were simply young and that their jets would eventually reach greater distances.

Now, in three different papers in The Astrophysical Journal, a Caltech-led team of researchers has concluded that CSOs are not young but relatively short-lived.

This image taken by VLBA shows the CSO named J1734+0926. The red spots are the edges of a strong dipole jet ejected from an unseen black hole. Credit: ML Lister/Purdue University
This image taken by VLBA shows the CSO named J1734+0926. The red spots are the edges of a strong dipole jet ejected from an unseen black hole. Credit: ML Lister/Purdue University

"These CSOs are not young," explains Prof. Emeritus Tony Redhead who headed the study. "You can't call a 12-year-old dog young even though it lives a shorter life than an adult person. These objects are their own type that lives and dies within thousands of years and not millions of years as is common in galaxies with larger jets."

In the new studies, the team reviewed the literature and past observations of 3,000 CSO candidates, verified 64 as genuine and identified 15 additional CSOs. All of these objects have previously been observed with the Very Large Array (VLBA), and some have been observed with other high-resolution radio telescopes. "The VLBA observations are the most detailed in astronomy, providing images with details equivalent to measuring the width of a human hair from a distance of 160 km," says Redhead.

This figure shows how CSOs are probably formed. When one massive star gets too close to a black hole (left), it is devoured. This causes the black hole to emit a very fast dipole jet (center). The jet extends outward and its hot edges glow with radio wave emissions (right). Credit: B. Saxton/NRAO/AUI/NSF
This figure shows how CSOs are probably formed. When one massive star gets too close to a black hole (left), it is devoured. This causes the black hole to emit a very fast dipole jet (center). The jet extends outward and its hot edges glow with radio wave emissions (right). Credit: B. Saxton/NRAO/AUI/NSF

The conclusion from the team's analysis is that CSOs emit jets for 5,000 years or less and then die out. "The CSO jets are very energetic jets, but they seem to be running out," says Vikram Ravi of Calcutta. "The jets stop flowing from the source".

As for what fuels the short-lived jets, scientists believe it's a tidal rip event (TDE), which occurs when a single massive star gets too close to a supermassive black hole and is devoured.

This image taken by VLBA shows two supermassive black holes, which appear as blobs with red streaks. Black holes are at the center of an elliptical galaxy. The colors represent different spectral gradients in radio emission, with red showing the densest regions around the black holes. The black hole on the right must have recently devoured a massive star, causing it to emit two very fast jets. The edges of these jets appear as green spots above and below the black hole. This object, named J0405+3803, is called a CSO because its jets are relatively close (or compact) compared to other black holes with much larger jets. Credit: HL Maness/Grinnell College
This image taken by VLBA shows two supermassive black holes, which appear as blobs with red streaks. Black holes are at the center of an elliptical galaxy. The colors represent different spectral gradients in radio emission, with red showing the densest regions around the black holes. The black hole on the right must have recently devoured a massive star, causing it to emit two very fast jets. The edges of these jets appear as green spots above and below the black hole. This object, named J0405+3803, is called a CSO because its jets are relatively close (or compact) compared to other black holes with much larger jets. Credit: HL Maness/Grinnell College

More of the topic in Hayadan:

2 תגובות

  1. He is interesting and helps me to understand a problem in physics that I am researching about the connection between the heat map and another interesting phenomenon.

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